Discovery | |
---|---|
Discovered by | Auguste Charlois |
Discovery date | 7 December 1896 |
Designations | |
(423) Diotima | |
Pronunciation | /daɪ.əˈtaɪmə/[1] |
Named after | Diotima of Mantinea (Διοτίμα Diotīma) |
1896 DB | |
Main belt | |
Adjectives | Diotimean /daɪ.ɒtəˈmiːən/, Diotimian /daɪ.əˈtɪmiən/ |
Orbital characteristics[2] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 116.96 yr (42719 d) |
Aphelion | 3.18523 AU (476.504 Gm) |
Perihelion | 2.95026 AU (441.353 Gm) |
3.06774 AU (458.927 Gm) | |
Eccentricity | 0.038297 |
5.37 yr (1962.6 d) | |
237.495° | |
0° 11m 0.355s / day | |
Inclination | 11.2304° |
69.4710° | |
200.103° | |
Physical characteristics | |
Dimensions | 171 km × 138 km[3] |
175.859±3.854 km[2] 211.64 ± 16.02 km[4] | |
Mass | (6.91±1.93)×1018 kg[4] (4.368 ± 1.680/1.377)×1018 kg[5] |
Mean density | 1.39 ± 0.50 g/cm3[4] 1.534 ± 0.590/0.483 g/cm3[5] |
4.775 h (0.1990 d)[2] | |
0.067±0.015[2] | |
C[2] | |
7.42[2] | |
423 Diotima is one of the larger main-belt asteroids. It is classified as a C-type asteroid[2] and is probably composed of primitive carbonaceous material.
It was discovered by Auguste Charlois on 7 December 1896, in Nice. In the late 1990s, a network of astronomers worldwide gathered lightcurve data that was ultimately used to derive the spin states and shape models of 10 new asteroids, including 423 Diotima. The light curve for this asteroid varies "a lot" depending on the position, with the brightness variations ranging from almost zero to up to 0.2 in magnitude.[6][7] Dunham (2002) used 15 chords and obtained an estimated size of 171 km × 138 km.[3]
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